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Shock Cooling Emission from Extended Material Revisited

Piro, Anthony L. and Haynie, Annastasia and Yao, Yuhan (2021) Shock Cooling Emission from Extended Material Revisited. Astrophysical Journal, 909 (2). Art. No. 209. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20210325-124223453

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Abstract

Following shock breakout, the emission from an astrophysical explosion is dominated by the radiation of shock-heated material as it expands and cools, known as shock cooling emission (SCE). The luminosity of SCE is proportional to the initial radius of the emitting material, which makes its measurement useful for investigating the progenitors of these explosions. Recent observations have shown some transient events have especially prominent SCE, indicating a large radius that is potentially due to low-mass extended material. Motivated by this, we present an updated analytic model for SCE that can be utilized to fit these observations and learn more about the origin of these events. This model is compared with numerical simulations to assess its validity and limitations. We also discuss SN 2016gkg and SN 2019dge, two transients with large early luminosity peaks that have previously been attributed to SCE of extended material. We show that their early power-law evolution and photometry are well matched by our model, strengthening support for this interpretation.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/abe2b1DOIArticle
https://arxiv.org/abs/2007.08543arXivDiscussion Paper
ORCID:
AuthorORCID
Piro, Anthony L.0000-0001-6806-0673
Yao, Yuhan0000-0001-6747-8509
Additional Information:© 2021 The American Astronomical Society. Received 2020 July 15; revised 2021 January 15; accepted 2021 February 1; published 2021 March 19. A.L.P. acknowledges financial support for this research from a Scialog award made by the Research Corporation for Science Advancement. A.H. acknowledges support from the USC-Carnegie fellowship. Y.Y. thanks the Heising-Simons Foundation for financial support.
Funders:
Funding AgencyGrant Number
Research CorporationUNSPECIFIED
University of Southern CaliforniaUNSPECIFIED
Carnegie InstitutionUNSPECIFIED
Heising-Simons FoundationUNSPECIFIED
Subject Keywords:Radiative transfer; Supernovae
Issue or Number:2
Classification Code:Unified Astronomy Thesaurus concepts: Radiative transfer (1335); Supernovae (1668)
Record Number:CaltechAUTHORS:20210325-124223453
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210325-124223453
Official Citation:Anthony L. Piro et al 2021 ApJ 909 209
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:108558
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Mar 2021 22:56
Last Modified:25 Mar 2021 22:56

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